List of exoplanets discovered in 2019

This list of exoplanets discovered in 2019 is a list of confirmed exoplanets that were first observed during 2019.[1][2]

For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.

Name Mass (MJ) Radius (RJ) Period (days) Semi-major axis (AU) Temp. (K)[3] Discovery method Distance (ly) Host star mass (M) Host star temp. (K) Remarks
7 Canis Majoris c 0.87 996.00 2.153 radial vel. 64.6 1.34 4826
Beta Pictoris c 9 1200 2.7 radial vel. 64.43 1.76
CI Tauri b 11.6+2.9
2.7
8.9891±0.0202 radial vel. 515.3±3.9 0.90±0.02
DS Tucanae Ab 0.509±0.015 8.138268±0.000011 850 transit 143.89±0.22 1.01±0.06 5428±80
Epsilon Indi Ab 3.25 16510 11.55 64.25 radial vel. 11.87 0.75
Gliese 49 b 0.0177+0.0021
0.0021
13.8508+0.0053
0.0051
0.0905±0.0011 radial vel. 32.145±0.01 0.515±0.019 3805±51
Gliese 143 b 0.09637+0.00827
0.00840
0.2280839±0.0282262 35.589+0.006
0.005
0.1932±0.0002 transit 53.25±0.02 0.76+0.03
0.02
Gliese 357 b 0.00579 0.1086 3.93072 0.035 525 transit 30.80 0.342 3505
Gliese 357 c 0.0107 9.1247 0.061 401.2 radial vel. 30.80 0.342 3505
Gliese 357 d 0.019 55.661 0.204 219.6 radial vel. 30.80 0.342 3505 Potentially habitable exoplanet
Gliese 378 b 0.04097 ± 0.006 3.822±0.001 0.082±0.002 radial vel. 48.79 0.56±0.01 3879±67
Gliese 411 b 0.00941±0.00145 12.9532±0.0079 349.83±0.32 radial vel. 8.284 0.386±0.039 3563±60
Gliese 685 b 0.028+0.0053
0.0057
24.160+0.061
0.047
0.1344+0.0052
0.0051
radial vel. 46.7102 0.3816±0.069 0.55±0.06
Gliese 686 b 0.022±0.003 15.53209+0.00166
0.00167
0.091±0.004 379+24
25
radial vel. 26.612±0.008 0.42±0.05 3663±68
Gliese 4276 b 0.05213+0.00296
0.00299
13.352±0.003 0.082±0.002 radial vel. 69.6±0.1 0.41±0.03 3387±51
HAT-P-69b 3.58 1.676 4.7869491 0.06555 1930 transit 1122 1.65 7394
HAT-P-70b <6.78 1.87 2.74432452 0.04739 2562 transit 1073 1.89 8450
HATS-54b 0.76 1.067 2.5441828 0.03763 1625 transit 2510 1.10 5702
HATS-55b 0.921 1.251 4.2042001 0.05412 1367 transit 2034 1.20 6214
HATS-56b 0.602 1.688 4.324799 0.06043 1902 transit 1882 1.57 6536
HATS-57b 3.147 1.139 2.3506210 0.03493 1413.4 transit 913 1.03 5587
HATS-58Ab 1.03 1.095 4.2180896 0.05798 1721 transit 1605 1.46 7175
HATS-70b 12.9+1.8
1.6
1.384+0.079
0.074
1.8882378±0.0000015 0.03632+0.00074
0.00087
2730+140
160
transit 4263+196
202
0.81+0.50
0.33
1.08+0.16
0.14
HD 1397 b 0.415±0.020 1.026+0.025
0.027
11.53533+0.00079
0.00080
0.1097+0.0011
0.0013
1228.3+10.0
9.9
transit 260.121 1.324+0.042
0.046
5521±60
HD 2685 b 1.17±0.12 1.44±0.05 4.12688+0.00005
0.00004
0.0568±0.0006 2061±28 transit 645.72+2.77
2.28
1.43+0.05
0.04
6801±76
HD 8326 b 0.210±0.062 158.991±1.440 0.533±0.011 radial vel. 100.2 0.80±0.05 4914+51
32
HD 13724 b 26.77+4.40
2.20
14763.405+4901.655
1599.795
12.40+2.60
0.90
radial vel. 141.9±0.17 0.76±0.71 5868±27
HD 15337 b 0.0236+0.0034
0.0032
0.146±0.005 4.75615±0.00017 0.0522±0.0012 1001.0±11.5 transit 146.36±0.23 0.90±0.03 5125±50
HD 15337 c 0.0255+0.0057
0.0053
0.213±0.011 17.1784±0.0016 0.1268±0.0038 642±10 transit 146.36±0.23 0.90±0.03 5125±50
HD 20003 b 0.0367±0.0033 0.2051 11.8482+0.0016
0.0017
0.0974+0.0034
0.0039
radial vel. 142.86±4.08 0.88 5494±27
HD 20003 c 0.0454+0.0046
0.0044
0.2103 33.9239+0.0239
0.0266
0.1964+0.0068
0.0078
radial vel. 142.86±4.08 0.88 5494±27
HD 20781 d 0.0334+0.0038
0.0037
29.158+0.0102
0.01
0.1647+0.0076
0.0083
radial vel. 115.36±4.4 0.7 5256±29
HD 20781 e 0.0442±0.0049 85.5073+0.0983
0.0947
0.3374+0.0155
0.017
radial vel. 115.36±4.4 0.7 5256±29
HD 21411 b 0.207±0.081 84.288±0.127 0.362±0.007 radial vel. ±95.11 0.89±0.05 5605+247
132
HD 21693 b 0.0259+0.0034
0.0033
0.1976 22.6786+0.0085
0.0087
0.1455+0.0058
0.0063
radial vel. 105.61±1.66 0.8 5430±26
HD 21693 c 0.0547±0.0056 53.7357+0.0312
0.0309
0.2586+0.0103
0.0113
radial vel. 105.61±1.66 0.8 5430±26
HD 21749 c <0.0116 0.0796+0.0057
0.0052
7.78993+0.00051
0.00044
0.0695+0.0021
0.0023
701+25
23
transit 53.261±0.023 0.73±0.07 4640±100
HD 23472 b 0.05638+0.00444
0.04405
17.667+0.142
0.095
0.121±0.001 transit 127.46±0.13 0.75+0.04
0.03
HD 23472 c 0.05405+0.00337
0.04333
29.625+0.224
0.171
0.170±0.001 transit 127.46±0.13 0.75+0.04
0.03
HD 24085 b 0.0371±0.0098 2.0455±0.0002 0.034±0.001 radial vel. 179.4 1.22±0.07 6034+32
53
HD 25015 b 4.48+0.30
0.28
6019.320+679.365
262.980
6.19+0.45
0.23
radial vel. 122.2±0.22 0.86±0.05 5160±63
HD 31527 b 0.0329±0.0028 16.5535+0.0034
0.0035
0.1254+0.0041
0.0045
radial vel. 125.8±2.9 0.96 5898±13
HD 31527 c 0.0445±0.0040.0039 51.2053+0.0373
0.0368
0.2663+0.0088
0.0095
radial vel. 125.8±2.9 0.96 5898±13
HD 31527 d 0.0372+0.0053
0.0052
271.6737+2.1135
2.2471
0.8098+0.0273
0.0293
radial vel. 125.8±2.9 0.96 5898±13
HD 39855 b 0.027±0.005 3.2498±0.0004 0.041±0.001 radial vel. 75.93 0.87±0.05 5576+50
46
HD 45184 b 0.0384+0.0033
0.0032
5.8854±0.0003 0.0644+0.002
0.0021
radial vel. 71.36±0.62 1.03 5869±14
HD 45184 c 0.0277+0.0034
0.0032
13.1354+0.0026
0.0025
0.11+0.0034
0.0036
radial vel. 71.36±0.62 1.03 5869±14
HD 51608 b 0.0402+0.0038
0.0037
14.0726±0.0016 0.1059+0.0043
0.0046
radial vel. 113.6±2.02 0.8 5358±22
HD 51608 c 0.045+0.0051
0.0048
95.9446+0.1555
0.1366
0.3809+0.0153
0.0164
radial vel. 113.6±2.02 0.8 5358±22
HD 64114 b 0.0560±0.0110 45.791±0.070 0.246±0.005 radial vel. 102.9 0.95±0.05 5676+32
87
HD 65216c 1.295±0.062 577.6±1.328 1.301±0.020 radial vel. 114.7±0.1 0.95±0.01 5718±8 Rediscovered in 2019 after false positive in 2013[4]
HD 92788 c 3.67+0.30
0.25
11611.2975+5055.06
905.820
10.50+2.90
0.55
radial vel. 113.1385 1.15±0.07 5744±24
HD 92987 b 16.88+0.69
0.65
10354.8375+551.5275
270.2850
9.62+0.36
0.26
radial vel. 142.2±0.22 1.08±0.06 5770±36
HD 97048 b 2.5 130 imaging 603 2.4 10000 Discovered using study of disk kinematics
HD 102843 b 0.3584±0.0456 3090.942±295.049 4.074±0.270 radial vel. 205.05 0.95±0.05 5436+144
69
HD 103949 b 0.0352±0.0072 120.878±0.446 0.439±0.009 radial vel. 86.50 0.77±0.04 4792+66
54
HD 125390 b 22.16 1756.2 3.16 radial vel. 503 1.36 4850
HD 180617 b 0.03839+0.00315
0.0044
105.9+0.09
0.1
0.3357+0.0099
0.01
radial vel. 19.28±0.07 0.45±0.04 3557±51
HD 181234 b 8.37+0.34
0.36
7462.0575+80.3550
76.7025
12.40+2.60
0.90
radial vel. 155.9±0.42 1.01±0.06 5386±60
HD 202772 Ab 1.017+0.070
0.068
1.545+0.052
0.060
3.308958±0.000083 0.05208+0.00064
0.00068
2132+28
30
transit 480.1+8.2
7.8
1.72+0.06
0.07
6272+77
71
HD 206255 b 0.108±0.022 96.045±0.317 0.461±0.009 radial vel. 245.9 1.42±0.08 5635+82
99
HD 210193 b 0.4817±0.0733 649.918±8.599 1.487±0.031 radial vel. 137.8 1.04±0.06 5790+38
50
HD 211970 b 0.0409±0.0079 25.201±0.025 0.143±0.003 radial vel. 42.4 0.61±0.04 4127+149
94
HD 213885 b 0.0278+0.0021
0.0020
0.1557+0.0045
0.0046
1.008035+0.000021
0.000020
0.02012+0.00015
0.00012
transit 156.45721±0.4566189 1.068+0.020
0.018
5978±50 A transiting 1-day-period super-Earth with an Earth-like composition around a bright (V=7.9) star unveiled by TESS
HD 213885 c 0.06277+0.00434
0.00428
4.78503+0.00056
0.000051
0.056798+0.00044
0.00032
1265.4+7.3
8.4
radial vel. 156.45721±0.4566189 1.068+0.020
0.018
5978±50
HD 219666 b 0.0522±0.0041 0.420±0.015 6.03607+0.00064
0.00063
0.06356±0.00265 1073±20 transit 307.98 1.03±0.03 5527±65
HD 220197 b 0.20 1728 2.729 radial vel. 210 0.91 5683
HD 221416 b 0.190±0.018 0.836+0.031
0.028
14.2767±0.0037 0.1228+0.00025
0.00026
transit 310.0931 1.212±0.074 5080±90 Hot Saturn-type planet confirmed by TESS
HD 221420 b 9.70+1.10
1.00
22482+4200
4100
18.5±2.3 radial vel. 101.7±0.12 1.67±0.11 5830±44
HD 233832 b 1.78 2058 2.827 radial vel. 192 0.71 4981
HIP 35173 b 0.0400±0.0085 41.516±0.077 0.217±0.004 radial vel. 108.25 0.79±0.05 4881+55
81
HIP 54373 b 0.02712±0.00579 7.760±0.003 0.063±0.001 radial vel. 61.09 0.57±0.03 4021+226
146
HIP 54373 c 0.03914±0.00664 15.144±0.008 0.0990±0.0020 radial vel. 61.09 0.57±0.03 4021+226
146
HIP 71135 b 0.0592±0.0129 87.190±0.381 0.335±0.007 radial vel. 105.5 0.66±0.04 4146+107
110
HIP 79098 (AB)b 20.5±4.5 345±6 2450±150 imaging 477.2±8.2 3.75±1.25 Brown dwarf
HR 858 b 0.1860+0.0061
0.0057
3.58599±0.00015 0.0480+0.0010
0.0011
1572+22
19
transit 104.35 1.145+0.074
0.080
6201±50
HR 858 c 0.1730±0.0062 5.97293+0.00060
0.00053
0.0674+0.0014
0.0016
1326+18
16
transit 104.35 1.145+0.074
0.080
6201±50
HR 858 d 0.1931+0.0077
0.0074
11.2300+0.0011
0.0010
0.1027+0.0022
0.0025
1075+15
13
transit 104.35 1.145+0.074
0.080
6201±50
HR 5183 b 3.23 27000 18 171 radial vel. 102.7 1.07 5794 Exoplanet found with one of the most elliptical orbits as of 2019
K2-32e 0.0901+0.0089
0.008
4.34882+0.00069
0.00075
0.04951±0.00055 transit 516.6±4.2 0.856±0.028 With a radius almost identical to that of the Earth it is almost certainly a terrestrial planet
K2-43c 0.216 2.198884 1093.7 transit 598 0.57 3841
K2-50c 0.089+0.011
0.01
3.96151+0.00046
0.00051
transit 845.82±10.63 0.61±0.06
K2-63c 0.35±0.11 25.4556±0.0047 0.189±0.011 transit 524.414±21 1.40±0.25 6771±303
K2-133e 0.154+0.012
0.012
26.5841+0.0018
0.0017
0.1346±0.0011 296±10 transit 245.3±0.7 0.46±0.01 3655±80
K2-146c 0.02358 0.195 4.00498 1093.7 transit 259 0.33 3385
K2-166c 0.109+0.019
0.015
3.80464+0.00091
0.00105
transit 1568.81+31.64
29.03
1.07±0.03
K2-168c 0.105+0.012
0.009
8.0468+0.0024
0.0025
transit 800.91±13.67 0.91±0.03
K2-198c 0.1270 3.3596055 1229.9 transit 362 0.80 5213
K2-198d 0.2175 7.4500177 943.2 transit 362 0.80 5213
K2-282c 0.132+0.012
0.009
0.70531±0.00005 transit 1638.22±25.34 0.94±0.04 5499±109 3rd planet discovered in 2020[5]
K2-290b 0.0664 0.273±0.014 9.21165+0.00033
0.00034
0.0923±0.0066 1230±38 transit 897±12 1.19+0.07
0.08
6302±120
K2-290c 0.774±0.047 1.006±0.050 48.36685+0.00041
0.00040
0.0923±0.0066 676±16 transit 897±12 1.19+0.07
0.08
6302±120
K2-291b 0.0204±0.0036 0.1418+0.0085
0.0064
2.225177+0.000066
0.000068
0.03261±0.00044 transit 295±2 0.93±0.04 5520±60
K2-292b 0.0771±0.0138 0.235+0.010
0.009
16.9841±0.0008 0.13±0.01 795+33
28
transit 372.76+2.67
2.64
1.00±0.03 5725±65
K2-293b 0.219+0.031
0.022
13.1225+0.0011
0.0012
750+170
50
transit 1290±22 0.96+0.04
0.03
5532±78
K2-294b 0.148+0.019
0.017
2.50387+0.00022
0.00023
1425+79
54
transit 1230±20 0.99+0.03
0.03
5612±50
K2-295b 0.335±0.062 {0.897+0.011
0.005
4.024867±0.000015 0.0451+0.0006
0.0014
852+14
6
transit 736.1±7.8 0.74±0.04 4444±70
K2-296b 0.167+0.018
0.04
28.1656+0.0027
0.0028
transit 521.78±4.57 0.41+0.11
0.05
K2-297b 0.062+0.005
0.004
2.13174±0.00022 transit 831.31±5.48 0.78+0.09
0.17
K2-298b 0.098+0.012
0.011
4.16959+0.00051
0.00053
transit 1441.42±26.65 0.8+0.08
0.16
K2-299b 0.152+0.053
0.028
4.50756+0.00062
0.0006
transit 1219.21±16.28 0.93+0.08
0.1
5724±72 Two more planets in star system discovered in 2020[5]
K2-300b 0.09+0.021
0.012
2.87814+0.00023
0.00026
transit 528.67±5.87 0.22+0.04
0.06
K2-301b 0.145+0.015
0.017
5.29711+0.00074
0.0007
transit 1491.42±44.98 0.56±0.05 4114±99
K2-302b 0.08+0.017
0.018
2.25372±0.00047 transit 359.49±3.52 0.41+0.1
0.08
Two more planets in system discovered in 2020[5]
K2-303b 0.086+0.01
0.013
1.58252+0.00017
0.00018
transit 1034.57±9.59 0.71+0.09
0.03
K2-304b 0.118+0.007
0.008
2.28943±0.00019 transit 1380.78±23.94 0.83+0.09
0.12
K2-305b 0.194+0.06
0.037
18.0983+0.006
0.0058
transit 2030.88±33.92 1.11+0.14
0.12
K2-306b 0.143+0.012
0.014
34.885+0.011
0.01
transit 931.54±6.69 0.91+0.04
0.16
K2-307b 0.1+0.011
0.008
15.2841+0.0037
0.0029
transit 1053.09±20.65 0.95±0.04
K2-308b 0.884±0.087 3.38628±0.00002 transit 1.09±0.09 6100±263
K2-310b 0.2307±0.0112 13.6030±0.0013 0.0980±0.0040 536±18 transit 1133.22 0.690±0.038 4684±79
K2-310c 0.2400±0.0130 65.5500±0.0089 0.280±0.006 316±10 transit 1133.22 0.690±0.038 4684±79
K2-311b <13 1.11±0.07 3650+1280
1130
4.5±1.0 183+25
18
transit 1826.48 0.90±0.09 4898±68
KELT-23Ab 0.938+0.048
0.044
1.323±0.025 2.255251+0.000011
0.000012
0.03302+0.00068
0.00064
1561±20 transit 409.07±1.14 0.94+0.06
0.05
5899±49
KELT-24b 5.18 1.272 5.5514926 0.06969 1459 transit 313.2 1.46 6509
Kepler-47d 0.05984+0.07501
0.03672
0.628+0.059
0.044
187.366+0.069
0.051
0.6992+0.0031
0.0033
transit 4900 0.957+0.013
0.015
Kepler-65e 0.653+0.056
0.055
258.8+1.5
1.3
0.362±0.007 radial vel. 999.3±8.8 1.25±0.06 6211±66
Kepler-82f 0.0658±0.0031 75.732±0.012 0.3395±0.0041 timing 3026.64 0.91±0.03 5401±108
Kepler-448c 22 2500 4.2 timing 1318 1.5
Kepler-1658b 5.88 1.04 3.8494 0.0546 transit 2629.05 2.891+0.130
0.106
6216±78 First exoplanet candidate detected by Kepler Space Telescope (known as KOI-4.01), confirmed in 2019.
Kepler-1659b 0.028±0.001 0.17±0.02 13.608±0.00006 0.11229 transit 3812.7570 1.02
Kepler-1659c 0.0014±0.001 0.17±0.03 20.4415±0.0013 0.1472 transit 3812.7570 1.02
Kepler-1660b 7.693±0.054 237.68977±0.08237 timing 4013.68±73.27 1.21 This detection arose from a search for eclipse timing variations among the more than 2,000 eclipsing binaries observed by Kepler.
KMT-2016-BLG-0212Lb 18 2.2 microlensing 21000 0.48
KMT-2016-BLG-1107Lb 3.283+3.468
1.835
0.342+0.070
0.085
microlensing 21700+3090
4400
0.087+0.092
0.049
KMT-2017-BLG-0165Lb 0.11+0.05
0.04
3.45+0.98
0.95
microlensing 14774.88 0.760+0.340
0.270
[6][7]
KMT-2017-BLG-1038Lb 2.0+2.0
1.1
1.8+0.6
0.5
microlensing 19569.3826 0.37+0.36
0.20
KMT-2017-BLG-1146Lb 0.710+0.800
0.420
1.6±0.6 microlensing 21200.16 0.33+0.36
0.20
KMT-2018-BLG-1990Lb 0.348 0.763 microlensing 3150 0.09
LHS 3844 b 0.1162±0.0020 0.46292913±0.00000190 0.00622±0.00017 805±20 transit 48.60±0.03 0.15±0.01 3036±77
LP 791-18 b 0.0999 0.9480050 0.009690 650 transit 86.41 0.14 2960
LP 791-18 c 0.206 4.989963 0.029392 370 transit 86.41 0.14 2960
Luyten 98-59 b 0.00157+0.00094
0.00063
0.071±0.004 2.25314±0.00002 0.0233±0.0017 transit 34.64 0.31±0.01 {3367±150
Luyten 98-59 c 0.00755+0.00566
0.00252
0.12+0.007
0.006
3.690621+0.000013
0.000014
0.0324±0.0023-0.0024 transit 34.64 0.31±0.01 3367±150
Luyten 98-59 d 0.0107+0.0085
0.0044
0.14±0.012 7.45086+0.00004
0.00005
0.052±0.004 transit 34.64 0.31±0.01 3367±150
LSPM J2116+0234 b 0.04185+0.00315
0.00346
14.4399+0.0078
0.0087
0.0876+0.0022
0.0021
radial vel. 57.53±0.07 0.43±0.03 3475±51
LTT 1445 Ab 0.0069 0.123 5.35882 0.03807 433 transit 22.4 0.26 3337 [8]
MOA-bin-29b 0.600 0.48 microlensing 23200 0.03
NGTS-4b 0.0648±0.0094 0.284±0.023 1.3373508±0.0000080 0.019±0.005 1650±400 transit 921.7±5.9 0.75±0.02 5143±100
NGTS-5b 0.229±0.037 1.136±0.023 3.3569866±0.0000026 0.0382±0.0013 952±24 transit 309.5±8.5 0.66+0.07
0.06
4987±41
NGTS-6b 1.339 1.326 0.8820590 0.01677 transit 1010 0.77 4730
NGTS-8b 0.93 1.09 2.49970 0.035 1345 transit 1420 0.89 5241
NGTS-9b 2.90 1.07 4.43527 0.058 1448 transit 1420 1.34 6330
NSVS 14256825 b 14.15±0.16 3225±22 3.12±0.07 timing 2734.2±137.31 0.42±0.07 40000
NY Virginis c 5.54 8799 timing 1800
OGLE-2015-BLG-1649L 2.54 2.07 microlensing 1380 0.34
OGLE-2015-BLG-1670Lb 0.0563+0.0302
0.0277
2.62+0.58
0.60
microlensing 22000+3300
4200
0.55±0.28
OGLE-2016-BLG-1067Lb 0.43 1.70 microlensing 3730 0.30
OGLE-2018-BLG-0596Lb 0.04383±0.00491 0.97±0.13 microlensing 18400±2400 0.23±0.03
OGLE-2018-BLG-0740Lb 4.8 5480 6.1 microlensing 10400 1.0 5912
OGLE-2018-BLG-1011Lb 1.8 6.1 microlensing 23000 0.18
OGLE-2018-BLG-1011Lc 2.8 0.80 microlensing 23000 0.18
PDS 70b 8.0±6.0 >1.3 43500 22 imaging 369.96±1.70 0.76±0.02 3972±36
PDS 70c 8.0±4.0 34.5±2 imaging 369.96±1.7 0.76±0.02 3972±36
Qatar-6b 0.668 1.062 3.506195 0.0423 transit 330 0.822 5052
Qatar-7b 1.88±0.25 1.70±0.03 {2.0320460±0.0000097 0.0352±0.0002 transit 2364.6337 1.409±0.026 6387±38
Qatar-8b 0.371±0.062 1.285±0.022 3.71495±0.00100 0.0474±0.0008 1457±14 transit 902.5±11 1.03±0.05 5738±51
Qatar-9b 1.19±0.16 1.009±0.014 1.540731±0.000038 0.0234±0.0003 1134±9 transit 689.5±5.2 0.72±0.02 4309±31
Qatar-10b 0.736±0.090 1.543±0.040 1.645321±0.000010 0.0286±0.0006 1955±25 transit 1760±33 1.16±0.07 6124±46
SDSS J1228+1040 b 0.0009+0.0045
0.000758
0.0857±0.00021 0.0034±0.000009 1800 timing 413.337977±0.4892346 0.705±0.05 The smallest known exoplanet discovered.
Teegarden b 0.00330+0.00041
0.00038
4.9100±0.0014 0.0252+0.0008
0.0009
radial vel. 12.50±0.013 0.09±0.01 2904±51
Teegarden c 0.00349+0.00050
0.00047
11.409±0.009 0.0443+0.0014
0.0015
226 radial vel. 12.50±0.013 0.09±0.01 2904±51 Potentially habitable exoplanet
TOI-125 b 0.0299±0.00277 0.2432±0.00669 4.65382±0.00033 0.05186+0.00086
0.00077
1037±11 transit 363.3382±1.435088 0.859+0.044
0.038
5320±39 [9][10]
TOI-125 c 0.02086±0.00311 0.24614±0.009 9.15059+0.0007
0.00082
0.814±0.0013 827.8±8.6 transit 363.3382±1.435088 0.859+0.044
0.038
5320±39 [11][10]
TOI-125 d 0.0428±0.0038 0.2614±0.0152 19.98+0.005
0.0056
0.05186+0.00086
0.00077
638.1±6.6 transit 363.3382±1.435088 0.859+0.044
0.038
5320±39 [12][10]
TOI-150b 1.75+0.14
0.17
1.38±0.04 5.857342+0.000065
0.000066
0.0583+0.0013
0.0018
1493+29
32
transit 1095.89±6.52 1.25+0.07
0.12
6003+104
98
TOI-163b 1.22 1.489 4.231306 0.0580 1669 transit 1359 1.44 6495
TOI-172b 5.42+0.22
0.20
0.965+0.032
0.029
9.47725+0.00064
0.00079
0.0914±0.0017 transit 1097.418 1.128+0.065
0.061
5645±50
TOI-216b 0.094+0.063
0.044
0.686+0.145
0.074
17.089+0.011
0.015
0.1293+0.0067
0.0051
628+13
11
transit 583.30+2.9
2.9
0.87+0.04
0.03
5026±125
TOI-216c 0.63+0.53
0.31
1.007+0.052
0.037
34.556+0.014
0.010
0.2069+0.0107
0.0082
497+10
8
transit 583.30±2.9 0.87+0.04
0.03
5026±125
TOI-270b 0.0050 0.1112 3.360080 0.0306 528 transit 73.23 0.40 3386 [13][14]
TOI-270c 0.0193 0.216 5.660172 0.0472 424 transit 73.23 0.40 3386 [13][14]
TOI-270d 0.0150 0.190 11.38014 0.0733 340 transit 73.23 0.40 3386 [13][14]
TOI-564b 1.463+0.10
0.096
1.02+0.71
0.29
1.651144±0.000018 0.02734+0.00061
0.00053
1714+20
21
transit 643.8±5.9 0.998+0.068
0.057
5640+34
37
[15]
TOI-905b 0.667+0.042
0.041
1.171+0.052
0.051
3.739494±0.000038 0.04666+0.00096
0.0011
1192+39
36
transit 489.9+23.5
22.5
0.968+0.061
0.068
5570+150
140
[15]
V1298 Tauri b 0.911+0.049
0.053
24.13861+0.00102
0.00090
0.1687+0.0025
0.0026
668±22 transit 353.9±2.3 1.10±0.05 4970±120 [16]
V1298 Tauri c 0.499 8.24958 0.0825 845±27 transit 353.9 1.10 4970 [17]
V1298 Tauri d 0.572 12.4032 0.1083 677±22 transit 353.9 1.10 4970 [17]
V1298 Tauri e 0.780 60 0.308 492+66
104
transit 353.9 1.10 4970 [17]
WASP-18Ac 0.174±0.039 2.1558 0.035 timing 404 1.22 6400
WASP-126c 0.202±0.077 7.63±0.17 timing 763.206±48.9235 1.12 5800
WASP-166b 0.101±0.005 0.63±0.03 5.443540±0.000004 0.0641±0.0011 1270±30 transit 368.55 1.19±0.06 6050±50
WASP-169b 0.561 1.304 5.6114118 0.0681 1604 transit 2080 1.34 6110
WASP-171b 1.084 0.980 3.8186244 0.05040 1642 transit 2530 1.17 5965
WASP-175b 0.990 1.208 3.0652907 0.04403 1571 transit 2080 1.21 6229
WASP-177b 0.508±0.038 1.58+0.66
0.83
3.071722±0.000001 0.03957±0.00058 1142±32 transit 580.5583 0.876±0.038 5017±70
WASP-178b 1.66 1.81 3.3448285 0.0558 2470 transit 1360 2.07 9360 [18]
WASP-180Ab 0.9 1.24 3.409264 0.048 transit 830 1.3 6600
WASP-181b 0.299±0.034 1.184+0.071
0.059
4.159±0.0000034 0.00542±0.00069 1186+32
26
transit 1444.872 1.04±0.04 5839±70
WASP-182b 0.148 0.850 3.3769848 0.0451 1479 transit 1080 1.08 5638
WASP-183b 0.502±0.047 1.47+0.94
0.33
4.11177±0.0000051 0.0463±0.00075 1111±30 transit 1069.79292 1.00±0.03 0.784±0.038
WASP-184b 0.57 1.33 5.18170 0.0627 1480 transit 2090 1.23 6000 [18]
WASP-185b 0.980 1.25 9.38755 0.0904 1160 transit 897 1.12 5900 [18]
WASP-190b 1.0±0.1 1.15±0.09 5.367753±0.000004 0.0663±0.0008 1500±50 transit 1796.323 1.35±0.05 6400±100
WASP-192b 2.30 1.23 2.8786765 0.0408 1620 transit 1610 1.09 5910 [18]
KMT-2016-BLG-1836L b 2.2+1.9
1.1
3.5+1.1
0.9
microlensing 23157.1+2609.25
7827.753
0.49+0.38
0.25
[19]
HD 85628 A b 3.1±0.9 1.53+0.07
0.04
2.82406±0.00003 0.047±0.004 2100±100 transit 559.47±3.05 1.75±0.05 7800±200 Mascara-4b: A3V giant star and a planet on retrograde orbit.[20]
OGLE-2016-BLG-1227 b 0.79+1.3
0.39
3.4+2.1
1
microlensing 0.1+0.17
0.05
[21]
OGLE-2013-BLG-0911L b 9.51+2.72
1.69
microlensing 10500+1500
1100
0.29+0.07
0.05
[22]
L 1159-16 b 0.088+0.060
0.035
241.59+4.6
4.0
0.403+0.039
0.047
radial vel. 14.584±0.007 0.15 3158 [23][24]
L 1159-16 c 0.222+0.083
0.068
766.954+16.710
19.237
0.871+0.087
0.100
radial vel. 14.584±0.007 0.15 3158 [23][24]

Specific exoplanet lists

References

  1. "NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. California Institute of Technology. Retrieved 27 March 2018.
  2. "Extrasolar Planet's Catalogue (sic)". Kyoto University. Retrieved 20 December 2019.
  3. "The Extrasolar Planets Encyclopaedia". Retrieved 20 January 2018.
  4. Wittenmyer, Robert A.; et al. (2019). "Truly eccentric – I. Revisiting eight single-eccentric planetary systems". Monthly Notices of the Royal Astronomical Society. 484 (4): 5859–5867. arXiv:1901.08471. Bibcode:2019MNRAS.484.5859W. doi:10.1093/mnras/stz290.
  5. ULTRA SHORT PERIOD PLANETS IN K2 III: NEIGHBORS ARE COMMON WITH 12 NEW MULTI-PLANET SYSTEMS AND 26 NEWLY VALIDATED PLANETS IN CAMPAIGNS 0-8, 10, 2020, arXiv:2011.11698
  6. KMT-2017-BLG-0165Lb: A Super-Neptune mass planet Orbiting a Sun-like Host Star, 2018, arXiv:1809.01288
  7. KMT-2017-BLG-2820 and the Nature of the Free-Floating Planet Population, 2020, arXiv:2010.07527
  8. THREE RED SUNS IN THE SKY: A TRANSITING, TERRESTRIAL PLANET IN A TRIPLE M DWARF SYSTEM AT 6.9 PARSECS, 2019, arXiv:1906.10147
  9. exoplanet.eu toi-125_b
  10. Mass determinations of the three mini-Neptunes transiting TOI-125, 2020, arXiv:2001.08834
  11. exoplanet.eu toi-125_c
  12. exoplanet.eu toi-125_d
  13. "太陽系外惑星「TOI 270 b、c、d」を発見。地球外生命体の存在は?". sorae. 2019-07-30. Retrieved 2021-01-08.
  14. Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley, 2021, arXiv:2101.01593
  15. Davis, Allen B.; Wang, Songhu; et al. (2020). "TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS". Astronomical Journal. 160: 229. arXiv:1912.10186. doi:10.3847/1538-3881/aba49d/pdf.
  16. A WARM JUPITER-SIZED PLANET TRANSITING THE PRE-MAIN SEQUENCE STAR V1298 TAU, 2019, arXiv:1902.09670
  17. Four newborn planets transiting the young solar analog V1298 Tau, 2019, arXiv:1910.04563
  18. WASP-South hot Jupiters: WASP-178b, WASP-184b, WASP-185b & WASP-192b, 2019, arXiv:1907.11667
  19. Yang, Hongjing; et al. (2020). "KMT-2016-BLG-1836Lb: A Super-Jovian Planet from a High-cadence Microlensing Field". The Astronomical Journal. 159 (3): 98. arXiv:1908.10011. Bibcode:2020AJ....159...98Y. doi:10.3847/1538-3881/ab660e.
  20. exoplanet.eu Planet OGLE-2016-BLG-1227 b
  21. exoplanet.eu Planet OGLE-2013-BLG-0911L b
  22. Barnes, J. R.; et al. (2019-06-11), Frequency of planets orbiting M dwarfs in the Solar neighbourhood, arXiv:1906.04644v1, Bibcode:2019arXiv190604644T.
  23. Search for Nearby Earth Analogs. III. Detection of ten new planets, three planet candidates, and confirmation of three planets around eleven nearby M dwarfs, 2020, arXiv:2008.07998
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